OGLEII high pm stars towards Galactic Centre (Rattenbury+, 2008)

Details OGLEII high pm stars towards Galactic Centre (Rattenbury+, 2008) OGLEII high pm stars towards Galactic Centre (Rattenbury+, 2008)

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73850905r&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/385/905. Originally published in: 2008MNRAS.385..905R

Computer Science

Stars: Nearby, Proper Motions, Photometry: Infrared, Stars: Distances

Scientific paper

The photometry data base of the second phase of the OGLE microlensing experiment, OGLE-II, is a rich source of information about the kinematics and structure of the Galaxy. In this work, we use the OGLE-II proper motion catalogue to identify candidate stars which have high proper motions. 521 stars with proper motion {mu}>50mas/yr in the OGLE-II proper motion catalogue were cross-identified with stars in the MACHO high proper motion catalogue, and the DEep Near-Infrared Survey and Two-Micron All-Sky Survey infrared photometry catalogues. Photometric distances were computed for stars with colours consistent with G/K- and M-type stars. Six stars were newly identified as possible nearby (<50pc) M dwarfs.
(3 data files).

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